The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise | Paper Citation Record

Observation 9ed2cd41-b5a6-49f1-bc4c-5e8dc1421d91 · outbound

This paper cites We use vw to denote the velocity of the bubble walls, and set vw = 1 to obtain a conservative estimation of ΩGW.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise We use vw to denote the velocity of the bubble walls, and set vw = 1 to obtain a conservative estimation of ΩGW

Reference 1

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Observation 6c8a61f3-1932-4c7a-9d16-8fd91a11f5c8 · outbound

This paper cites The peak frequency of GW energy spectrum can be estimated 6 as fp = 1.1×10−9Hz g∗(Tann) 10 1/2 × g∗s(Tann) 10 −1/3 Tann 10−2GeV.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The peak frequency of GW energy spectrum can be estimated 6 as fp = 1.1×10−9Hz g∗(Tann) 10 1/2 × g∗s(Tann) 10 −1/3 Tann 10−2GeV

Reference 2

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Observation a846214e-a0ba-4bfd-9c75-7e7cf68e94b5 · outbound

This paper cites an unresolved cited work.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Unresolved cited work

Reference 3

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Observation 09fad32c-8cd0-494a-b4ec-2501f90164c4 · outbound

This paper cites Stochastic background of gravitational waves from cosmological sources.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Stochastic background of gravitational waves from cosmological sources

Reference 4

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Observation d15df7fe-663c-4371-b547-ac18832ae206 · outbound

This paper cites Probing the Universe through the Stochastic Gravitational Wave Background.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Probing the Universe through the Stochastic Gravitational Wave Background

Reference 5

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Observation 5d6f3494-cdca-483e-89c2-4e79d21e5b34 · outbound

This paper cites Cosmological Backgrounds of Gravitational Waves.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Cosmological Backgrounds of Gravitational Waves

Reference 6

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Observation ca378ac0-eb94-4a3c-84fe-d8bfaa745f8c · outbound

This paper cites Stochastic Gravitational Wave Backgrounds.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Stochastic Gravitational Wave Backgrounds

Reference 7

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Observation dafe2d27-811a-4e41-a317-74f105be4718 · outbound

This paper cites Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects

Reference 8

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Observation fa14cdd4-d2d8-4375-9f9d-fd5183d93412 · outbound

This paper cites The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background

Reference 9

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Observation f44605f0-e3ee-438b-9a09-7f53f2e1778c · outbound

This paper cites The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars

Reference 10

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Observation ea212e78-3e28-45b2-8fe5-d915ca2a43d9 · outbound

This paper cites The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.694586Z

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Observation 75ae9511-69de-4eba-ac6b-1009f3c856f2 · outbound

This paper cites The second data release from the European Pulsar Timing Array I. The dataset and timing analysis.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The second data release from the European Pulsar Timing Array I. The dataset and timing analysis

Reference 12

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Observation 9322b158-9ed5-4dca-92e8-140ec713fc55 · outbound

This paper cites The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.718408Z

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Observation cffa2289-94b4-4420-9319-cf80451bc966 · outbound

This paper cites Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.727773Z

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Observation 6b5301e7-75f6-4113-b10e-7388aadc1e9e · outbound

This paper cites Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.949250Z

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Observation 2c406fe5-d471-45e7-bff0-6b36f8955bf3 · outbound

This paper cites The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.957786Z

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Observation f852978d-3310-49f4-a024-c94eddd6e23b · outbound

This paper cites Gravitational Waves from SMBH Binaries in Light of the NANOGrav 15-Year Data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Gravitational Waves from SMBH Binaries in Light of the NANOGrav 15-Year Data

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.969692Z

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Observation e4fec0aa-9dbb-43cb-842c-8c29138ca202 · outbound

This paper cites Dark Matter Spike surrounding Supermassive Black Holes Binary and the Nanohertz Stochastic Gravitational Wave Background.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Dark Matter Spike surrounding Supermassive Black Holes Binary and the Nanohertz Stochastic Gravitational Wave Background

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.979538Z

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Observation 076021a1-9a42-41fe-9295-4155403eb064 · outbound

This paper cites Probing the Dark Matter density with gravitational waves from super-massive binary black holes.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Probing the Dark Matter density with gravitational waves from super-massive binary black holes

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.985294Z

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Observation 8b55335a-958f-4477-8098-7f2363dfd87b · outbound

This paper cites Implications for the Supermassive Black Hole Binaries from the NANOGrav 15-year Data Set.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Implications for the Supermassive Black Hole Binaries from the NANOGrav 15-year Data Set

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:42.995259Z

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Observation 223d00b4-d3ed-42f0-9e5a-4c830a4a3bf3 · outbound

This paper cites Detecting new fundamental fields with Pulsar Timing Arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Detecting new fundamental fields with Pulsar Timing Arrays

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.007896Z

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Observation cdcd28ab-513a-41d0-ba90-5e168416d163 · outbound

This paper cites NANOGrav Signal from a Dark Conformal Phase Transition.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise NANOGrav Signal from a Dark Conformal Phase Transition

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.017075Z

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Observation 80edcdad-13d0-4a63-9dcb-7e797ec200c1 · outbound

This paper cites Have pulsar timing array methods detected a cosmological phase transition?.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Have pulsar timing array methods detected a cosmological phase transition?

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.027833Z

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Observation 30433485-3667-4a9f-a2c4-c6a01b604b64 · outbound

This paper cites Pulsar Timing Array Stochastic Background from light Kaluza-Klein resonances.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Pulsar Timing Array Stochastic Background from light Kaluza-Klein resonances

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.033742Z

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Observation d0f7f96a-74ef-4e46-9fc4-bfe9af028efe · outbound

This paper cites Implications of Nano-Hertz Gravitational Waves on Electroweak Phase Transition in the Singlet Dark Matter Model.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Implications of Nano-Hertz Gravitational Waves on Electroweak Phase Transition in the Singlet Dark Matter Model

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.042177Z

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Observation 1d2c683c-6b66-4e24-bdfd-05846d200023 · outbound

This paper cites A collider test of nano-Hertz gravitational waves from pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise A collider test of nano-Hertz gravitational waves from pulsar timing arrays

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.048835Z

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Observation dcd52cf5-dd22-46e6-9bd9-334b0791949b · outbound

This paper cites Heavy QCD axion model in light of pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Heavy QCD axion model in light of pulsar timing arrays

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.055303Z

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Observation c77272ae-d3f7-4e75-9c06-7a1aa5476314 · outbound

This paper cites First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.064082Z

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Observation d0028d87-6322-4eb3-9966-93ede59d0e32 · outbound

This paper cites Axionic domain walls at Pulsar Timing Arrays: QCD bias and particle friction.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Axionic domain walls at Pulsar Timing Arrays: QCD bias and particle friction

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.082762Z

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Observation cc8123be-95dd-4d50-86d2-ab3472ed7e65 · outbound

This paper cites Scale of Dirac leptogenesis and left-right symmetry in the light of recent PTA results.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Scale of Dirac leptogenesis and left-right symmetry in the light of recent PTA results

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.101382Z

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Observation f804f64a-2a2c-4d9e-95d9-7e3538e27826 · outbound

This paper cites NANOGrav spectral index $\gamma=3$ from melting domain walls.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise NANOGrav spectral index $\gamma=3$ from melting domain walls

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.108785Z

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Observation 4792cbd4-91ca-4267-a96f-1530f15ebfb5 · outbound

This paper cites Catastrogenesis with unstable ALPs as the origin of the NANOGrav 15 yr gravitational wave signal.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Catastrogenesis with unstable ALPs as the origin of the NANOGrav 15 yr gravitational wave signal

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.116280Z

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Observation 070cca09-b4c6-44a1-ba6f-622e54469805 · outbound

This paper cites Nano-Hertz gravitational waves from collapsing domain walls associated with freeze-in dark matter in light of pulsar timing array observations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Nano-Hertz gravitational waves from collapsing domain walls associated with freeze-in dark matter in light of pulsar timing array observations

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.125287Z

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Observation 21d71f63-4304-41d6-80ef-c0ddad007e18 · outbound

This paper cites Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data

Reference 34

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Observation 862b277f-855e-49f7-9cd8-9227770bfe98 · outbound

This paper cites Nanohertz gravitational waves from cosmic strings and dark photon dark matter.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Nanohertz gravitational waves from cosmic strings and dark photon dark matter

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.144212Z

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Observation 841b6d70-5bfa-4769-8691-923aa1b46d5b · outbound

This paper cites The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.152438Z

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Observation 2de2edae-f3a7-45b1-812a-4e7ccf72a68b · outbound

This paper cites Superheavy quasi-stable strings and walls bounded by strings in the light of NANOGrav 15 year data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Superheavy quasi-stable strings and walls bounded by strings in the light of NANOGrav 15 year data

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.162975Z

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Observation 9b45f2fe-a4cc-4d4a-b23c-3103e6a53ebc · outbound

This paper cites From quantum gravity to gravitational waves through cosmic strings.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise From quantum gravity to gravitational waves through cosmic strings

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.184174Z

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Observation 3e8c1bd3-3bca-4d58-b811-d5b287adda1a · outbound

This paper cites Dark baryon from pure Yang-Mills theory and its GW signature from cosmic strings.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Dark baryon from pure Yang-Mills theory and its GW signature from cosmic strings

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.195712Z

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Observation de4c24d6-6a5f-4514-bbaf-6c8a58b3ce0a · outbound

This paper cites The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.226553Z

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Observation 64188841-4136-4b26-aeb1-bb7e82bf95df · outbound

This paper cites Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.241153Z

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Observation 2abdf6df-daec-4503-8aff-8ee8d5edf626 · outbound

This paper cites The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.247784Z

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Observation 0e521564-3061-4793-83e3-f3ee02d5e8d0 · outbound

This paper cites Limits on scalar-induced gravitational waves from the stochastic background by pulsar timing array observations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Limits on scalar-induced gravitational waves from the stochastic background by pulsar timing array observations

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.255580Z

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Observation d1d34330-d6ec-4486-a7e9-ddd8d5301254 · outbound

This paper cites Implications for the non-Gaussianity of curvature perturbation from pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Implications for the non-Gaussianity of curvature perturbation from pulsar timing arrays

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.264012Z

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Observation 21f36aed-d6f6-4936-9dbb-150b7b29af6f · outbound

This paper cites Translating nano-Hertz gravitational wave background into primordial perturbations taking account of the cosmological QCD phase transition.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Translating nano-Hertz gravitational wave background into primordial perturbations taking account of the cosmological QCD phase transition

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.271903Z

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Observation ef6ccec1-1725-4f89-96de-d9e2629e22da · outbound

This paper cites Scalar induced gravitational waves in light of Pulsar Timing Array data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Scalar induced gravitational waves in light of Pulsar Timing Array data

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.278021Z

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Observation 1f10f2e5-0698-45e9-bf14-411a5078262e · outbound

This paper cites Induced Gravitational Waves from Ultra Slow-Roll Inflation and Pulsar Timing Arrays Observations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Induced Gravitational Waves from Ultra Slow-Roll Inflation and Pulsar Timing Arrays Observations

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.284343Z

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Observation 0aee89c4-80b8-4b49-9ad7-a4137b935910 · outbound

This paper cites Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.298878Z

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Observation 3a81440e-7f7f-4be1-95a5-afebf3328ebe · outbound

This paper cites Constraints on primordial curvature power spectrum with pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Constraints on primordial curvature power spectrum with pulsar timing arrays

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.305849Z

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Observation 5c5a4acb-8cbb-493f-a9ca-71bc5b2ab550 · outbound

This paper cites Can the gravitational wave background feel wiggles in spacetime?.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Can the gravitational wave background feel wiggles in spacetime?

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.313716Z

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Observation df045ffb-24f4-44ba-ac9d-75031be62125 · outbound

This paper cites PBHs and GWs from $\mathbb{T}^2$-inflation and NANOGrav 15-year data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise PBHs and GWs from $\mathbb{T}^2$-inflation and NANOGrav 15-year data

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.322905Z

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Observation 3d5deb63-2cb5-48f1-aef4-bfdea60b7137 · outbound

This paper cites Scalar-induced gravitational wave interpretation of PTA data: the role of scalar fluctuation propagation speed.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Scalar-induced gravitational wave interpretation of PTA data: the role of scalar fluctuation propagation speed

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.330379Z

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Observation 37c9c4c7-8a66-4f90-b4a6-2576692093d4 · outbound

This paper cites Confronting sound speed resonance with pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Confronting sound speed resonance with pulsar timing arrays

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.338621Z

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Observation 1a4d49db-2a50-4556-b39a-0bde5fa9d0be · outbound

This paper cites Gravitational wave background from quintessential inflation and NANOGrav data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Gravitational wave background from quintessential inflation and NANOGrav data

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.350466Z

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Observation ac732a4b-2a7c-4eee-a24c-064dd052c1a7 · outbound

This paper cites Probing The Early Universe Cosmology With NANOGrav: Possibilities and Limitations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Probing The Early Universe Cosmology With NANOGrav: Possibilities and Limitations

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.360074Z

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Observation 7da03f32-ab2c-4d73-810b-c183eb6beaf1 · outbound

This paper cites Probing the equation of state of the early Universe with pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Probing the equation of state of the early Universe with pulsar timing arrays

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.367776Z

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Observation 959272a6-5bbf-4077-b0fc-94abaf3bfd45 · outbound

This paper cites Model-independent reconstruction of the primordial curvature power spectrum from PTA data.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Model-independent reconstruction of the primordial curvature power spectrum from PTA data

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.374592Z

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Observation 94860a74-b3b6-4d91-b303-ddf2622f546f · outbound

This paper cites On the inflationary interpretation of the nHz gravitational-wave background.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise On the inflationary interpretation of the nHz gravitational-wave background

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.387015Z

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Observation 0c7adab9-fa88-406d-a20f-aef3af51c135 · outbound

This paper cites Ultra-low mass PBHs in the early universe can explain the PTA signal.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Ultra-low mass PBHs in the early universe can explain the PTA signal

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.402740Z

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Observation daa49899-27ad-4e4b-b913-cebc16135d61 · outbound

This paper cites Full analysis of the scalar-induced gravitational waves for the curvature perturbation with local-type non-Gaussianities.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Full analysis of the scalar-induced gravitational waves for the curvature perturbation with local-type non-Gaussianities

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.418784Z

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Observation a3b73561-e12b-412c-b418-bec324b374a6 · outbound

This paper cites Extra-tensor-induced origin for the PTA signal: No primordial black hole production.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Extra-tensor-induced origin for the PTA signal: No primordial black hole production

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.431216Z

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Observation 30d8eb61-8171-4c05-b4f5-45bacc438cf0 · outbound

This paper cites The NANOGrav 15-year Data Set: Search for Signals from New Physics.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The NANOGrav 15-year Data Set: Search for Signals from New Physics

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.441420Z

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Observation 02e510e4-0a21-4b4e-b113-819789baa156 · outbound

This paper cites What is the source of the PTA GW signal?.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise What is the source of the PTA GW signal?

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.454694Z

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Observation 4b0cb3c9-76be-4290-a65e-5aa7984c494a · outbound

This paper cites Probing Primordial Stochastic Gravitational Wave Background with Multi-band Astrophysical Foreground Cleaning.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Probing Primordial Stochastic Gravitational Wave Background with Multi-band Astrophysical Foreground Cleaning

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-08-15T20:02:45.971668Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 7b1dd7b0-ebff-4330-a715-8e0b818a4333 · outbound

This paper cites Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.490063Z

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Observation 53bb82e9-ad6a-4adc-a2ab-f7cf0b9a0441 · outbound

This paper cites Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.498922Z

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Observation 1b810e55-19ec-4625-86af-36e824d05175 · outbound

This paper cites Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.506818Z

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Observation dfdceb5d-4801-4d2e-8850-0798170a4770 · outbound

This paper cites Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.518267Z

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Observation 4e90085d-cb6a-4b3c-b4df-33e922e66e11 · outbound

This paper cites Impact of LIGO-Virgo black hole binaries on gravitational wave background searches.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Impact of LIGO-Virgo black hole binaries on gravitational wave background searches

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-08-15T20:02:45.774369Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 2fb39d25-2fcb-43bb-a8cd-7fbfe007313a · outbound

This paper cites Numerical simulations of acoustically generated gravitational waves at a first order phase transition.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Numerical simulations of acoustically generated gravitational waves at a first order phase transition

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.535243Z

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Observation 75f8d65e-ac0a-4cff-8b09-d834e16c43a0 · outbound

This paper cites Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.544818Z

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Observation db8b43f5-e5ab-4d75-bf26-7849d59f3842 · outbound

This paper cites Magnetic field and gravitational waves from the first-order Phase Transition.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Magnetic field and gravitational waves from the first-order Phase Transition

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.559532Z

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Observation 243f1f69-a755-47cd-b712-2e16676a9287 · outbound

This paper cites On the estimation of gravitational wave spectrum from cosmic domain walls.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise On the estimation of gravitational wave spectrum from cosmic domain walls

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.570000Z

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Observation b8e5a6d3-a3d4-4a4f-90b3-2ca1f0dd096a · outbound

This paper cites an unresolved cited work.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Unresolved cited work

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.582024Z

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Observation 93ebdde0-e8eb-4a04-8d15-d95822019e42 · outbound

This paper cites Liu, Phys.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Liu, Phys

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.587333Z

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Observation 1ab87c78-5b9b-4872-8453-e162ac11d8a1 · outbound

This paper cites WIMPs and new physics interpretations of the PTA signal are incompatible.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise WIMPs and new physics interpretations of the PTA signal are incompatible

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.602969Z

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Observation f59491dd-a8b5-40eb-a636-e16d5f859574 · outbound

This paper cites Are ultracompact minihalos really ultracompact?.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Are ultracompact minihalos really ultracompact?

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.614052Z

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Observation 6f3816ce-6717-4087-8680-9debe73c4692 · outbound

This paper cites Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.622128Z

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Observation 3bdc67f4-7042-4f03-8e68-0248beca7c1e · outbound

This paper cites Improved constraints on the primordial power spectrum at small scales from ultracompact minihalos.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Improved constraints on the primordial power spectrum at small scales from ultracompact minihalos

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.639101Z

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Observation cc6a5029-1e94-41bb-87b0-194f9ad6766f · outbound

This paper cites Expected properties of the first gravitational wave signal detected with pulsar timing arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Expected properties of the first gravitational wave signal detected with pulsar timing arrays

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.649878Z

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Observation a69e6aab-db91-4485-bf21-5ab9d0164780 · outbound

This paper cites Punturo et al.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Punturo et al

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.664135Z

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Observation ef1eb53a-b2a6-4c81-b7bb-6b852ad67181 · outbound

This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.679533Z

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Observation 8aa8dda4-c04a-4f68-925f-b6b63cfe4b58 · outbound

This paper cites Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.695234Z

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Observation 832f6e44-95bf-4295-b953-e2446b6a1769 · outbound

This paper cites Detecting gravitational waves from cosmological phase transitions with LISA: an update.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Detecting gravitational waves from cosmological phase transitions with LISA: an update

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.703087Z

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Observation 5c8a2ea0-f85e-4071-8155-00db787cacb8 · outbound

This paper cites Gravitational waves from a first order electroweak phase transition: a brief review.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Gravitational waves from a first order electroweak phase transition: a brief review

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.713666Z

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Observation a04d5b68-6eef-4962-a497-ad60d093fce8 · outbound

This paper cites Cosmic phase transitions: their applications and experimental signatures.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Cosmic phase transitions: their applications and experimental signatures

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.719663Z

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Observation 7c65f7d1-811d-4f3e-b454-8f1ac0af7b5d · outbound

This paper cites Constraining first-order phase transitions with curvature perturbations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Constraining first-order phase transitions with curvature perturbations

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.733314Z

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Observation f44d7c63-4725-44a2-abeb-ab4bb4a57951 · outbound

This paper cites Primordial Black Holes from Sound Speed Resonance during Inflation.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Primordial Black Holes from Sound Speed Resonance during Inflation

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.744668Z

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Observation b1275a01-08b3-4e19-9d70-6b93a6d3963e · outbound

This paper cites Primordial black holes and gravitational waves from parametric amplification of curvature perturbations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Primordial black holes and gravitational waves from parametric amplification of curvature perturbations

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.755794Z

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Unavailable: canonical work link unavailable.

Observation 3a551cab-6db8-4864-9b27-3db8be0ef541 · outbound

This paper cites A review of gravitational waves from cosmic domain walls.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise A review of gravitational waves from cosmic domain walls

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.773141Z

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Observation 1197ff30-c193-4f5f-b086-d14dd875c926 · outbound

This paper cites The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.786156Z

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Unavailable: canonical work link unavailable.

Observation 0cda139f-421e-4f95-8992-ccbd535b2bf5 · outbound

This paper cites Gravitational wave astronomy with the SKA.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Gravitational wave astronomy with the SKA

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.792752Z

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Observation 161c21a3-8171-4651-89f2-c545edc68a90 · outbound

This paper cites Inflation and Primordial Black Holes.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Inflation and Primordial Black Holes

Reference 93

Resolution: malformed identifier; no resolver link, observed 2026-08-15T20:02:43.800884Z

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Observation 242c673f-c509-42cc-9fd7-d7397bddf079 · outbound

This paper cites an unresolved cited work.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Unresolved cited work

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.808908Z

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Observation 7423a6c3-b559-410c-a274-9b61dc561164 · outbound

This paper cites Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.824285Z

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Observation 7a0281e0-cd69-4444-a831-843c48607ea0 · outbound

This paper cites A Cosmological Signature of the SM Higgs Instability: Gravitational Waves.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise A Cosmological Signature of the SM Higgs Instability: Gravitational Waves

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.835527Z

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Observation 18eee497-5ed5-43a5-b6ea-655f94637b3d · outbound

This paper cites Lensing constraints on ultradense dark matter halos.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Lensing constraints on ultradense dark matter halos

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.842318Z

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Unavailable: canonical work link unavailable.

Observation edf0a23b-a3b6-43d2-b20b-994fec2b8a96 · outbound

This paper cites Ultradense dark matter haloes accompany primordial black holes.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Ultradense dark matter haloes accompany primordial black holes

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.850975Z

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Observation e6ebc178-7491-492c-8c9c-d789936c38ff · outbound

This paper cites On Features and Nongaussianity from Inflationary Particle Production.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise On Features and Nongaussianity from Inflationary Particle Production

Reference 99

Resolution: verified exact; local_arxiv, observed 2026-08-15T20:02:44.653707Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation e31e6f69-e668-4363-b100-6a385620fbcd · outbound

This paper cites Primordial black holes and stochastic gravitational wave background from inflation with a noncanonical spectator field.

The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Primordial black holes and stochastic gravitational wave background from inflation with a noncanonical spectator field

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-15T20:02:43.877803Z

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